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These images from the Radar instrument aboard NASA’s Cassini spacecraft show the evolution of a transient feature in the large hydrocarbon sea named Ligeia Mare on Saturn’s moon Titan. Credit: NASA/JPL-Caltech/ASI/Cornell

NASA’s Cassini spacecraft has found deep, steep-sided canyons on Titan that are flooded with liquid hydrocarbons. The finding represents the first direct evidence of the presence of liquid-filled channels on Titan, as well as the first observation of canyons hundreds of meters deep. Scientists analyzed Cassini data from a close pass the spacecraft made over Titan in May 2013. During the flyby, Cassini’s radar focused on channels that branch out from the large, northern sea Ligeia Mare.

The Cassini observations reveal that the channels – in particular, a network of them na...